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- Ahmed El Goresy
- Max-Planck-Institut für Chemie, J.-Becher-Weg 27, D-55128 Mainz, Germany.
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- Leonid Dubrovinsky
- Theoretical Geochemistry Program, Institute of Earth Sciences, Uppsala University, S-75236, Uppsala, Sweden.
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- Thomas G. Sharp
- Department of Geology, Arizona State University, Tempe, AZ 85287, USA.
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- Surendra K. Saxena
- Theoretical Geochemistry Program, Institute of Earth Sciences, Uppsala University, S-75236, Uppsala, Sweden.
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- Ming Chen
- Guangzhou Institute of Geochemistry, Academia Sinica, Guangzhou 510640, China.
書誌事項
- 公開日
- 2000-06-02
- DOI
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- 10.1126/science.288.5471.1632
- 公開者
- American Association for the Advancement of Science (AAAS)
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説明
<jats:p> A post-stishovite phase of silica was identified in the Shergotty meteorite by x-ray diffraction and field emission scanning electron microscopy. The diffraction pattern revealed a monoclinic lattice, similar to the baddeleyite-structured polymorph with the cell parameters <jats:italic>a</jats:italic> = 4.375(1) angstroms, <jats:italic>b</jats:italic> = 4.584(1) angstroms, <jats:italic>c</jats:italic> = 4.708(1) angstroms, β= 99.97(3), ρ = 4.30(2) grams per cubic centimeter, where the numbers in parentheses are the maximum deviations. Transmission electron microscopy investigations indicate the presence of the α-lead dioxide–like polymorph, stishovite, and secondary cristobalite in the same silica grain. The mixture of high-density polymorphs suggests that several post-stishovite phases were formed during the shock event on the Shergotty parent body. </jats:p>
収録刊行物
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- Science
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Science 288 (5471), 1632-1634, 2000-06-02
American Association for the Advancement of Science (AAAS)
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詳細情報 詳細情報について
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- CRID
- 1362262944761269376
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- NII論文ID
- 80011836508
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- ISSN
- 10959203
- 00368075
- http://id.crossref.org/issn/00368075
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